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(gravitational wave*) OR gravitationswelle*

    Where do we stand in testing general relativity?

    Schäfer, G. | Elsevier | 2003
    gravity. Completed towards the end of 1915, until now the theory has passed all tests, including the prediction of gravitational waves. The paper ...

    VLBI for better gravimetry in SELENE

    Hanada, H. / Iwata, T. / Namiki, N. et al. | Elsevier | 2007
    improve the accuracy to which the low degree gravitational harmonics and the gravity field near the limb can be measured, and when combined with ...

    Ultralow-temperature resonant gravitational wave detectors, present state and future prospects

    Frossati, G. | Elsevier | 2003
    AbstractResonant gravitational wave detectors have evolved from the room ...

    The midlatitude ionosphere D-region response to some events on the sun

    Gokov, Alexander M. / Tyrnov, Oleg F. | Elsevier | 2002
    D-region. Such processes in this height range are accompanied by the generation and enhancement of acoustic-gravitational waves with periods ...

    The gravitational wave signature of young and dense star clusters

    Portegies Zwart, Simon F. | Elsevier | 2006
    gravitational wave radiation in the LISA band. If the star captured by the intermediate mass black hole is relatively low mass (≲2M ...
    Schlagwörter: Gravitational waves

    The final phase of inspiral of neutron stars: Realistic equations of state

    Gondek-Rosińska, D. / Bejger, M. / Bulik, T. et al. | Elsevier | 2006
    -shedding limit for neutron star binaries. The gravitational wave frequency at the ISCO, which marks the end of the inspiral phase, is found to be ...
    Schlagwörter: Gravitational waves

    The double-pulsar binary J0737–3039

    Lyne, A.G. | Elsevier | 2005
    detection of such events by the new ground-based gravitational wave detectors. ...

    The CHAMP-only earth gravity field model EIGEN-2

    Reigber, Ch / Schwintzer, P / Neumayer, K.-H et al. | Elsevier | 2003
    since July 2000 in a highly inclined orbit with an altitude of initially 450 km and meanwhile at about 400 km. From the gravitational orbit ...

    Spiral galaxies as gravitational plasmas

    Griv, E. / Gedalin, M. / Yuan, C. | Elsevier | 2004
    critical wavelength of the spiral structure arising due to nonresonant Jeans-type instability of gravity perturbations is explained. A formal ...
    Schlagwörter: Waves and instabilities

    Search of gravitational waves with resonant detectors

    Pizzella, G. | Elsevier | 1989
    Abstract The search for gravitational waves with the resonant bar ...

    Screening of Newtonian potential and dark matter problem

    Bashkirov, A.G. / Vityazev, A.V. | Elsevier | 2002
    characteristic wave number of the pair correlation function (PCF) k0 ∼ 0.05 h Mpc ...

    Possibilities for measurement and compensation of stray DC electric fields acting on drag-free test masses

    Weber, W.J. / Carbone, L. / Cavalleri, A. et al. | Elsevier | 2003
    ) gravitational wave mission. This paper proposes a simple technique to measure and compensate average stray DC potentials at the mV level, yielding ...
    Schlagwörter: Gravitational waves

    Position determination of gravitational wave sources with LISA

    Peterseim, M. / Jennrich, O. / Schutz, B.F. et al. | Elsevier | 2003
    observation of gravitational waves, currently under study by ESA. A brief introduction of the main features of this detector, concentrating on its one ...

    Performance of the Keck long wavelength spectrometer

    Campbell, R.D / Jones, B | Elsevier | 2003
    AbstractThe W.M. Keck Observatory’s Long Wavelength Spectrometer (LWS), is the ...
    Schlagwörter: Long Wavelength Spectrometer

    Performance of GPS-based accelerometry: CHAMP and GRACE

    van den IJssel, Jose / Visser, Pieter | Elsevier | 2006
    wavelengths are well determined and high-frequency accelerations, caused by e.g. geomagnetic storms, are not well recovered. ...
    Schlagwörter: Non-gravitational accelerations

    Neutron star oscillations and QPOs during magnetar flares

    Watts, Anna L. / Strohmayer, Tod E. | Elsevier | 2006
    , we provide an up to date summary of the observations and the theoretical framework, including a brief discussion of gravitational wave ...

    Measuring a binary's orientation with LISA

    Jennrich, O. / Peterseim, M. / Danzmann, K. et al. | Elsevier | 2003
    distinguish between different polarizational states of a gravitational wave. Therefore, we assume a binary as a source of a gravitational wave ...

    Masses of merging compact object binaries

    Gondek-Rosińska, Dorota / Bulik, Tomasz / Belczyński, Krzysztof | Elsevier | 2005
    in gravitational waves. We simulate the population of such binaries using the Star Track population synthesis code. We find that black hole ...
    Schlagwörter: Gravitational waves

    LISA satellite formation control

    Bik, J.J.C.M. / Visser, P.N.A.M. / Jennrich, O. | Elsevier | 2007
    consists of a triangular formation of three satellites aiming at detecting gravitational waves. In linear approximation the LISA satellites ...